Home > Conference Contributions & Seminars > Conference Talks > Contributed Talks > PROBA2/SWAP EUV images of the large-scale EUV corona up to 3 solar radii: Can we close the gap in coronal magnetic field structure between 1.3 and 2.5 solar radii? |
De Groof, A. ; Seaton, D.B. ; Rachmeler, L. A. ; Berghmans, D.
Talk presented at Joint American Astronomical Society/American Geophysical Union Triennial Earth-Sun Summit, meeting #1, #409.01 on 2015-xx-xx
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Conference Contributions & Seminars > Conference Talks > Contributed Talks
Royal Observatory of Belgium > Solar Physics & Space Weather (SIDC)
Solar-Terrestrial Centre of Excellence